A two-fluid analysis of the Kelvin-Helmholtz instability in the dusty layer of a protoplanetary disk: A possible path toward planetesimal formation through gravitational instability

Astrophysical Journal

Volumn 641, Issue 2 I, 2006, Pages 1131-1147

  Michikoshi, Shugo ^a   Inutsuka, Shu Ichiro ^a  

^a KYOTO UNIVERSITY   (Japan)

Author keywords

Instabilities; Planetary systems: formation; Turbulence

Indexed keywords

EID: 33745312737     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/499799     Document Type: Article

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